Calculation of coronal line intensities for boron-like ions

Details Calculation of coronal line intensities for boron-like ions Calculation of coronal line intensities for boron-like ions

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...87..233s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 87, Sept. 1983, p. 233-242.

Physics

5

Coronagraphs, Line Spectra, Luminous Intensity, Solar Corona, Sulfur, Atomic Excitations, Boron, Electron Impact, Electron Transitions, Molecular Ions, Radiative Transfer, Solar Physics, Transition Probabilities

Scientific paper

New atomic data (Saha and Trefftz, 1982a) have been used to calculate line intensities of S XII for the physical conditions found in the solar corona. They are compared with similar calculations for Si X (Saha and Trefftz, 1982b) and with published work. For the density sensitive intensity ratio I227/I218 the new values give the observed ratio (Malinovski and Heroux, 1973) for an electron density of log Ne = 8.5 which is more likely than the density deduced from the values of Flower and Nussbaumer (1975), log Ne ⪉ 7.

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